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Table B.1.

Dust continuum properties of the 125 z-GAL sources derived using the optically thin modified blackbody in Section 4. The best-fit values indicate the 50th percentile and their corresponding uncertainties; i.e., the 16th and 84th percentiles of the posterior likelihood distribution. μ is the magnification factor for the gravitationally lensed sources. (Only extract(1))

Source zspec β Tdust[K] log(μdust/M) log(LFIR/L)
HeLMS Sources

HeLMS-1 1.9047
HeLMS-3 1.4202
HeLMS-11 2.4829
HeLMS-12 2.3699
HeLMS-14 1.6169
HeLMS-16 2.8187
HeLMS-17 2.2978
HeLMS-19 4.6879
HeLMS-20 2.1947
HeLMS-21 2.7710
HeLMS-23 1.4888
HeLMS-24 4.9841
HeLMS-25 2.1404
HeLMS-26 2.6887
HeLMS-27 3.7620
HeLMS-28 2.5322
HeLMS-30 1.8197
HeLMS-31 1.9494
HeLMS-34 2.2714
HeLMS-35 1.6684
HeLMS-36 3.9802
HeLMS-37 2.7576
HeLMS-38 2.1898
HeLMS-39 2.7659
HeLMS-40 3.1420
HeLMS-41 2.3353
HeLMS-42 1.9558

Notes.

(1)

The full table is available at the Centre de Données de Strasbourg (CDS).

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